This paper addresses the Cosmological Constant Problem, also known as the Vacuum Catastrophe. It proposes that the massive discrepancy between predicted and observed vacuum energy arises from a lack of geometric filtering in standard models. Within the BQGF framework, vacuum fluctuations are constrained by the Baysüngür Filtering Function, which truncates high-energy modes at the fundamental scale limit of the ZV-Field, providing a natural resolution to the 10^120 error.